Magnetic field measurements from the solar probe

Details Magnetic field measurements from the solar probe Magnetic field measurements from the solar probe

Sep 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978clus.nasa..155t&link_type=abstract

In JPL A Close-up of the Sun p 155-158 (SEE N78-32964 23-92)

Physics

Magnetic Signatures, Solar Flux Density, Solar Magnetic Field, Solar Probes, Spaceborne Telescopes, Focal Plane Devices, High Resolution, Imaging Techniques, Magnetic Flux, Mission Planning, Spatial Distribution

Scientific paper

An optical system for the solar probe is described as well as its capability for improvements in spatial resolution. A magnetograph for measuring the elementary flux tube and obtaining vector geometry field geometry offers the possibility of looking for low contrast weak structure. With the probe's orbit passing over the pole, the structure of the polar field can be directly measured. The detector plane of the system receives a telecentric image of the objective. Because there is an aperture in this focal plane that can both move and change size, polarized line profiles can be obtained at arbitrary points with variable spatial resolution. The telescope microprocessor searches for the magnetic elements and then constructs the vector field.

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